Singularities as Solitons? Quantum Vacuum Architecture of Black Holes

Fuente: arXiv
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1. Verfasser: Erkul, Eren Erberk
Format: Preprint
Veröffentlicht: 2025
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author Erkul, Eren Erberk
author_facet Erkul, Eren Erberk
contents We propose that black holes are \emph{soliton-esque} objects, where gravitational collapse is balanced by quantum vacuum dispersion, modeled via \(R+αR^{2}\) gravity. Classical singularities are replaced by oscillating, finite-radius cores, thereby evading static no-go theorems. The event horizon is replaced by the \textit{Lamarina}, a surface of maximum redshift whose surface geometry yields Hawking-like radiation with corrections. The Raychaudhuri equations impose a Dyson-type ceiling on the maximum radiated power \((P_{\infty} \lesssim c^{5}/G)\), while effective field theory matching dictates a universal minimum Lamarina radius set by the dispersion scale.
format Preprint
id arxiv_https___arxiv_org_abs_2510_06428
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Singularities as Solitons? Quantum Vacuum Architecture of Black Holes
Erkul, Eren Erberk
General Relativity and Quantum Cosmology
We propose that black holes are \emph{soliton-esque} objects, where gravitational collapse is balanced by quantum vacuum dispersion, modeled via \(R+αR^{2}\) gravity. Classical singularities are replaced by oscillating, finite-radius cores, thereby evading static no-go theorems. The event horizon is replaced by the \textit{Lamarina}, a surface of maximum redshift whose surface geometry yields Hawking-like radiation with corrections. The Raychaudhuri equations impose a Dyson-type ceiling on the maximum radiated power \((P_{\infty} \lesssim c^{5}/G)\), while effective field theory matching dictates a universal minimum Lamarina radius set by the dispersion scale.
title Singularities as Solitons? Quantum Vacuum Architecture of Black Holes
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2510.06428